World's Best Scientists 2026 revealed!

D-Index & Metrics

Physics

D-Index
82
Citations
17459
World Ranking
2884
National Ranking
269

Magda Arnaboldi publication distribution in Physics in 2026

The chart shows the distribution of publications by all Research.com ranked scientists in the field of Physics in 2026. The highlighted bar marks where Magda Arnaboldi sits on this spectrum.

103–122 publications: 7 scientists 123–142 publications: 10 scientists 143–162 publications: 31 scientists 163–182 publications: 35 scientists 183–202 publications: 53 scientists 203–222 publications: 81 scientists 223–242 publications: 85 scientists 243–262 publications: 112 scientists 263–282 publications: 114 scientists 283–302 publications: 126 scientists 303–322 publications: 136 scientists 323–342 publications: 162 scientists 343–362 publications: 155 scientists 363–382 publications: 156 scientists 383–402 publications: 134 scientists 403–422 publications: 145 scientists 423–442 publications: 147 scientists 443–462 publications: 131 scientists 463–482 publications: 131 scientists 483–502 publications: 116 scientists 503–522 publications: 106 scientists 523–542 publications: 103 scientists 543–562 publications: 87 scientists 563–582 publications: 84 scientists 583–602 publications: 94 scientists 603–622 publications: 70 scientists 623–642 publications: 76 scientists 643–662 publications: 60 scientists 663–682 publications: 54 scientists 683–702 publications: 60 scientists 703–722 publications: 48 scientists 723–742 publications: 64 scientists 743–762 publications: 48 scientists 763–782 publications: 37 scientists 783–802 publications: 43 scientists 803–822 publications: 34 scientists 823–842 publications: 36 scientists 843–862 publications: 32 scientists 863–882 publications: 32 scientists 883–902 publications: 31 scientists 903–922 publications: 25 scientists 923–942 publications: 15 scientists 943–962 publications: 24 scientists 963–982 publications: 13 scientists 983–1,002 publications: 21 scientists 1,003–1,022 publications: 21 scientists 1,023–1,042 publications: 16 scientists 1,043–1,062 publications: 9 scientists 1,063–1,082 publications: 19 scientists 1,083–1,102 publications: 11 scientists 1,103–1,122 publications: 17 scientists 1,123–1,142 publications: 11 scientists 1,143–1,162 publications: 7 scientists 1,163–1,182 publications: 4 scientists 1,183–1,202 publications: 10 scientists 1,203–1,222 publications: 8 scientists 1,223–1,242 publications: 16 scientists 1,243–1,262 publications: 4 scientists 1,263–1,282 publications: 10 scientists 1,283–1,302 publications: 5 scientists 1,303–1,322 publications: 7 scientists 1,323–1,342 publications: 4 scientists 1,343–1,362 publications: 8 scientists 1,363–1,382 publications: 6 scientists 1,383–1,402 publications: 7 scientists 1,403–1,422 publications: 3 scientists 1,423–1,442 publications: 4 scientists 1,443–1,462 publications: 4 scientists 1,463–1,468 publications: 3 scientists 1,469+ publications: 100 scientists
103 publications 1,469+

This scientist: 397 publications — 37th percentile

37% of scientists in this discipline score the same or lower.

The last bar groups every scientist with 1,469 publications or more.

Magda Arnaboldi D-index placement in Physics in 2026

The chart shows the D-index (discipline H-index) distribution of Physics scientists ranked by Research.com in 2026. The highlighted bar marks where Magda Arnaboldi sits on this spectrum.

70–71 D-Index: 76 scientists 72–73 D-Index: 110 scientists 74–75 D-Index: 143 scientists 76–77 D-Index: 153 scientists 78–79 D-Index: 144 scientists 80–81 D-Index: 167 scientists 82–83 D-Index: 167 scientists 84–85 D-Index: 166 scientists 86–87 D-Index: 132 scientists 88–89 D-Index: 155 scientists 90–91 D-Index: 134 scientists 92–93 D-Index: 137 scientists 94–95 D-Index: 102 scientists 96–97 D-Index: 112 scientists 98–99 D-Index: 110 scientists 100–101 D-Index: 116 scientists 102–103 D-Index: 97 scientists 104–105 D-Index: 103 scientists 106–107 D-Index: 87 scientists 108–109 D-Index: 90 scientists 110–111 D-Index: 67 scientists 112–113 D-Index: 78 scientists 114–115 D-Index: 75 scientists 116–117 D-Index: 67 scientists 118–119 D-Index: 69 scientists 120–121 D-Index: 60 scientists 122–123 D-Index: 59 scientists 124–125 D-Index: 53 scientists 126–127 D-Index: 42 scientists 128–129 D-Index: 41 scientists 130–131 D-Index: 33 scientists 132–133 D-Index: 32 scientists 134–135 D-Index: 45 scientists 136–137 D-Index: 19 scientists 138–139 D-Index: 24 scientists 140–141 D-Index: 28 scientists 142–143 D-Index: 31 scientists 144–145 D-Index: 22 scientists 146–147 D-Index: 20 scientists 148–149 D-Index: 12 scientists 150–151 D-Index: 16 scientists 152–153 D-Index: 24 scientists 154–155 D-Index: 23 scientists 156–157 D-Index: 15 scientists 158–159 D-Index: 15 scientists 160–161 D-Index: 11 scientists 162–163 D-Index: 17 scientists 164–165 D-Index: 12 scientists 166–167 D-Index: 11 scientists 168–169 D-Index: 9 scientists 170–171 D-Index: 9 scientists 172–173 D-Index: 11 scientists 174–175 D-Index: 4 scientists 176–177 D-Index: 8 scientists 178–179 D-Index: 5 scientists 180–181 D-Index: 3 scientists 182–183 D-Index: 4 scientists 184 D-Index: 4 scientists 185+ D-Index: 99 scientists
70 D-Index 185+

This scientist: 82 D-Index — 24th percentile

24% of scientists in this discipline score the same or lower.

The last bar groups every scientist with 185 D-Index or more.

Overview

Magda Arnaboldi is affiliated with the European Southern Observatory in Germany. Their research primarily focuses on physics and astronomy, with an emphasis on astronomy and astrophysics. The body of work spans multiple topics, including astronomy and astrophysical research, stellar, planetary, and galactic studies, galaxies' formation, evolution, and phenomena, as well as astrophysics and star formation studies. Additional areas of interest include astronomical observations and instrumentation, gamma-ray bursts and supernovae, and adaptive optics with wavefront sensing.

The scientist's research output shows a strong presence in several subfields, such as astronomy and astrophysics, instrumentation, computational mechanics, general health professions, and atomic and molecular physics, and optics. This diverse scope reflects a comprehensive approach to their scientific inquiries.

Frequent co-authors in their publications include Johanna Hartke, Ortwin Gerhard, Chiara Spiniello, G. D'Ago, and Marilena Spavone. These collaborations have contributed to a substantial body of research work.

Magda Arnaboldi's publication record is associated mostly with the following venues: arXiv (Cornell University), Astronomy and Astrophysics, Proceedings of the International Astronomical Union, Monthly Notices of the Royal Astronomical Society, and Springer Link (Chiba Institute of Technology).

Selected recent papers authored or co-authored by Arnaboldi include:

  • Hic sunt dracones: Cartography of the Milky Way spiral arms and bar resonances with Gaia Data Release 2, 2020, Astronomy and Astrophysics
  • The stellar halos of ETGs in the IllustrisTNG simulations: The photometric and kinematic diversity of galaxies at large radii, 2020, Springer Link (Chiba Institute of Technology)
  • The stellar halos of ETGs in the IllustrisTNG simulations, 2021, Astronomy and Astrophysics
  • Galaxy populations in the Hydra I cluster from the VEGAS survey, 2022, Astronomy and Astrophysics
  • The first detection of ultra-diffuse galaxies in the Hydra I cluster from the VEGAS survey, 2020, Springer Link (Chiba Institute of Technology)

Best Publications

  • The VIMOS VLT deep survey. First epoch VVDS-deep survey: 11 564 spectra with 17.5 ≤ IAB ≤ 24, and the redshift distribution over 0 ≤ z ≤ 5

    O. Le Fèvre;G. Vettolani;B. Garilli;L. Tresse

  • A dearth of dark matter in ordinary elliptical galaxies

    Aaron J. Romanowsky;Nigel G. Douglas;Magda Arnaboldi;Konrad Kuijken

  • The GALEX-VVDS measurement of the evolution of the far-ultraviolet luminosity density and the cosmic star formation rate

    D. Schiminovich;D. Schiminovich;O. Ilbert;S. Arnouts;B. Milliard

  • The VIMOS-VLT Deep Survey: Evolution of the galaxy luminosity function up to z=2 in first epoch data

    O. Ilbert;L. Tresse;E. Zucca;S. Bardelli

  • The VIMOS VLT Deep Survey. Public release of 1599 redshifts to I AB ≤24 across the Chandra Deep Field South

    O. Le Fevre;G. Vettolani;S. Paltani;L. Tresse

  • The VIMOS-VLT deep survey - Evolution of the galaxy luminosity function up to z = 2 in first epoch data

    O. Ilbert;L. Tresse;E. Zucca;S. Bardelli

  • The GALEX VIMOS-VLT Deep Survey Measurement of the Evolution of the 1500 Å Luminosity Function

    S. Arnouts;D. Schiminovich;D. Schiminovich;O. Ilbert;L. Tresse

  • The importance of mergers for the origin of intracluster stars in cosmological simulations of galaxy clusters

    Giuseppe Murante;Giuseppe Murante;Martina Giovalli;Ortwin Gerhard;Magda Arnaboldi

  • The VVDS data reduction pipeline: introducing VIPGI, the VIMOS Interactive Pipeline and Graphical Interface

    M. Scodeggio;P. Franzetti;B. Garilli;A. Zanichelli

  • Discovery of 9 Ly alpha emitters at redshift z~3.1 using narrow-band imaging and VLT spectroscopy

    R. P. Kudritzki;R. H. Mendez;J. J. Feldmeier;R. Ciardullo

  • The VIMOS VLT Deep Survey: The build-up of the colour-density relation

    O. Cucciati;A. Iovino;C. Marinoni;O. Ilbert

  • Discovery of Nine Lyα Emitters at Redshift z ~ 3.1 Using Narrowband Imaging and VLT Spectroscopy*

    R-P Kudritzki;R-P Kudritzki;R-P Kudritzki;R H Mendez;J Feldmeier;Robin Ciardullo

  • The Kinematics of the Planetary Nebulae in the Outer Regions of NGC 4406

    M. Arnaboldi;K. C. Freeman;R. H. Mendez;M. Capaccioli

  • Kinematic properties of early-type galaxy haloes using planetary nebulae

    L. Coccato;O. Gerhard;M. Arnaboldi;M. Arnaboldi;P. Das

  • The VIMOS VLT Deep Survey: The build-up of the colour-density relation

    Olga Cucciati;Olga Cucciati;A. Iovino;C. Marinoni;C. Marinoni;O. Ilbert;O. Ilbert

  • The VVDS data reduction pipeline: introducing VIPGI, the VIMOS Interactive Pipeline and Graphical Interface

    M. Scodeggio;P. Franzetti;B. Garilli;A. Zanichelli

  • The Diffuse Light in Simulations of Galaxy Clusters

    G Murante;M Arnaboldi;O Gerhard;S Borgani

  • The VLA-VIRMOS Deep Field I. Radio observations probing the microJy source population

    M. Bondi. P. Ciliegi;G. Zamorani;L. Gregorini;G. Vettolani

  • The VIMOS VLT Deep Survey - Evolution of the luminosity functions by galaxy type up to z=1.5 from first epoch data

    E. Zucca;O. Ilbert;S. Bardelli;L. Tresse

  • The VIRMOS-VLT Deep Survey

    O. Le Fèvre;G. Vettolani;D. Maccagni;D. Mancini

Frequent Co-Authors

Ortwin Gerhard
Ortwin Gerhard Max Planck Society
Kenneth C. Freeman
Kenneth C. Freeman Australian National University
Aaron J. Romanowsky
Aaron J. Romanowsky San Jose State University
Konrad Kuijken
Konrad Kuijken Leiden University
H. J. McCracken
H. J. McCracken Institut d'Astrophysique de Paris
Christian Marinoni
Christian Marinoni Aix-Marseille University
D. Maccagni
D. Maccagni National Institute for Astrophysics
S. Bardelli
S. Bardelli National Institute for Astrophysics
Elena Zucca
Elena Zucca National Institute for Astrophysics
A. Iovino
A. Iovino National Institute for Astrophysics

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